Speaker
Celine Combet
(LPSC, Grenoble)
Description
In this talk, I will give an overview of the main properties and functionalities of
the CLUMPY code. CLUMPY performs a semi-analytical calculation of the γ-ray flux
astrophysical J-factor from dark matter annihilation/decay in the Galaxy, including
dark matter substructures. The code can be used in three modes: i) to draw skymaps
from the Galactic smooth component and/or the substructure contributions, ii) to
calculate the flux from a specific halo (that is not the Galactic halo, e.g. dwarf
spheroidal galaxies) or iii) to perform simple statistical operations from a list of
allowed DM profiles for a given object.
Primary author
Celine Combet
(LPSC, Grenoble)
